Absorption lines from C ii 1334Å, Fe ii 1608Å, and
Al ii 1670Å ions are detected in the SDSS spectrum with an
equivalent width of \(0.36 \pm 0.04\) Å, \(0.25 \pm 0.08\) Å, and
\(0.59\pm 0.09\) Å, respectively. Based on the strong correlation seen
between the rest-frame equivalent width of Si ii\(\lambda \) 1526
line and metallicity, we derive an upper limit on the metallicity of
log\( Z/Z_{\odot } < -1.58\)  from the observed \(3\sigma \)  upper limit of
0.34Å on Si ii\(\lambda \) 1526 equivalent width
[1]}, [2]}, [3]}. In
addition, we also derive a metallciity of \(\simeq -\) 2.13 based on
C ii\(\lambda \) 1334 line using the apparent optical depth
method. This limit also places the DLA just below the average
metallicity of the population at this redshift
[4]}, and well below the typical
metallicity of DLAs chosen for targetted searches towards enriched
systems, which typically select DLAs with log \( Z/Z_{\odot } > -1.0\) 
. To date, only one
other DLA host at this low metallicity, namely J\(2358+0149\)  with log
Z/Z\(\odot \)  \(\simeq -\) 1.7 derived based on Si II absorption, is
detected at small impact parameter of \(< 15\)  kpc
[5]}.
